Wormholes from beyond
arXiv:2412.11947 · doi:10.1140/epjc/s10052-025-14052-w
Abstract
In a brane-world context in which our universe would be a four-dimensional brane embedded into a five-dimensional spacetime or bulk, wormhole geometries are induced on branes. In this article, the Morris-Thorne wormhole and the Molina-Neves wormhole are obtained on the brane using the Nakas-Kanti approach, which starts from a regular five-dimensional spacetime to obtain known black hole and wormhole solutions on the four-dimensional brane. From the bulk perspective, these wormholes are five-dimensional solutions supported by an exotic fluid, but from the brane perspective, such objects are wormholes not supported by any fields or particles that live on the four-dimensional spacetime. Thus, the cause of these wormholes is the bulk influence on the brane.
11 pages, 6 figures. V2 with a different interpretation of the wormhole throat. Published in The European Physical Journal C
References in corpus (11)
- Traversable wormholes: Some simple examples
- Wormhole geometries in f(R) modified theories of gravity
- Modified-gravity wormholes without exotic matter
- Modelling wormholes in gravity
- A general class of braneworld wormholes
- General relativistic Poynting-Robertson effect to diagnose wormholes existence: static and spherically symmetric case
- Braneworld stars and black holes
- Rotating black holes in a Randall-Sundrum brane with a cosmological constant
- Wormholes in de Sitter branes
- Localized brane-world black hole analytically connected to an AdS boundary
- Five-dimensional regular black holes in a brane world
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- On the uplift of 4D wormholes in Braneworld models and their 5D structure
- Geodesic dynamics in brane-de Sitter wormholes
- Localized five-dimensional rotating brane-world black hole Analytically Connected to an to an AdS boundary
- Black holes and wormholes in Deser-Woodard gravity
- Embedding Wormholes and Dyonic Black Strings in Warped Braneworlds via Local Sum Rules